{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:2KKGCWCBNJYWDN4YDFYEY6ZG2O","short_pith_number":"pith:2KKGCWCB","schema_version":"1.0","canonical_sha256":"d2946158416a7161b79819704c7b26d3b9f5a3e15e3165977002451caeea6231","source":{"kind":"arxiv","id":"2110.06231","version":2},"attestation_state":"computed","paper":{"title":"The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alexander B. Gurvich, Cameron Trapp, Claude-Andre Faucher-Giguere, Dusan Keres, Philip Hopkins, Suoqing Ji, T. K. Chan","submitted_at":"2021-10-12T18:00:03Z","abstract_excerpt":"Cosmic rays (CRs) are an important component in the interstellar medium (ISM), but their effect on the dynamics of the disk-halo interface (< 10 kpc from the disk) is still unclear. We study the influence of CRs on the gas above the disk with high-resolution FIRE-2 cosmological simulations of late-type Lstar galaxies at redshift around zero. We compare runs with and without CR feedback (with constant anisotropic diffusion around 3e29 cm^2/s and streaming). Our simulations capture the relevant disk halo interactions, including outflows, inflows, and galactic fountains. Extra-planar gas in all o"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2110.06231","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-10-12T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"f6ab6f1daf04bbabc3dd465aa9a43014d0134b3fc57c2cf54b7cad4599c575bf","abstract_canon_sha256":"9426b815a04a93c4cf194cedbf3cf0a8601bcb5db16b060b0722ebe347909e0d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:50:12.288351Z","signature_b64":"J5sdbAi3wf312NUM7Rmcy9DNmEJsldv9RgELQprQCxYhvXzaP1ZOWR8sP9rAsQzymjtzBVnOtSRoQO9ZqlgnCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d2946158416a7161b79819704c7b26d3b9f5a3e15e3165977002451caeea6231","last_reissued_at":"2026-07-05T04:50:12.287941Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:50:12.287941Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alexander B. Gurvich, Cameron Trapp, Claude-Andre Faucher-Giguere, Dusan Keres, Philip Hopkins, Suoqing Ji, T. K. Chan","submitted_at":"2021-10-12T18:00:03Z","abstract_excerpt":"Cosmic rays (CRs) are an important component in the interstellar medium (ISM), but their effect on the dynamics of the disk-halo interface (< 10 kpc from the disk) is still unclear. We study the influence of CRs on the gas above the disk with high-resolution FIRE-2 cosmological simulations of late-type Lstar galaxies at redshift around zero. We compare runs with and without CR feedback (with constant anisotropic diffusion around 3e29 cm^2/s and streaming). Our simulations capture the relevant disk halo interactions, including outflows, inflows, and galactic fountains. Extra-planar gas in all o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2110.06231","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2110.06231/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2110.06231","created_at":"2026-07-05T04:50:12.287997+00:00"},{"alias_kind":"arxiv_version","alias_value":"2110.06231v2","created_at":"2026-07-05T04:50:12.287997+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2110.06231","created_at":"2026-07-05T04:50:12.287997+00:00"},{"alias_kind":"pith_short_12","alias_value":"2KKGCWCBNJYW","created_at":"2026-07-05T04:50:12.287997+00:00"},{"alias_kind":"pith_short_16","alias_value":"2KKGCWCBNJYWDN4Y","created_at":"2026-07-05T04:50:12.287997+00:00"},{"alias_kind":"pith_short_8","alias_value":"2KKGCWCB","created_at":"2026-07-05T04:50:12.287997+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06744","citing_title":"CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra","ref_index":118,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O","json":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O.json","graph_json":"https://pith.science/api/pith-number/2KKGCWCBNJYWDN4YDFYEY6ZG2O/graph.json","events_json":"https://pith.science/api/pith-number/2KKGCWCBNJYWDN4YDFYEY6ZG2O/events.json","paper":"https://pith.science/paper/2KKGCWCB"},"agent_actions":{"view_html":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O","download_json":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O.json","view_paper":"https://pith.science/paper/2KKGCWCB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2110.06231&json=true","fetch_graph":"https://pith.science/api/pith-number/2KKGCWCBNJYWDN4YDFYEY6ZG2O/graph.json","fetch_events":"https://pith.science/api/pith-number/2KKGCWCBNJYWDN4YDFYEY6ZG2O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O/action/storage_attestation","attest_author":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O/action/author_attestation","sign_citation":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O/action/citation_signature","submit_replication":"https://pith.science/pith/2KKGCWCBNJYWDN4YDFYEY6ZG2O/action/replication_record"}},"created_at":"2026-07-05T04:50:12.287997+00:00","updated_at":"2026-07-05T04:50:12.287997+00:00"}